A Model of One Proton Emission from Deformed Nuclei Jim Al-Khalili University of Surrey, UK PRESPEC Decay Physics Workshop University of Brighton, 12-13 January 2011

The Z≤82 Region Z=82 Stable N=82 N=104 Nuclei Thanks to D. T. Joss Au Pb Tl Re Hg Ir Os Lu Hf W Ta Pt Yb N=82 Stable Nuclei N=104 Proton emitter Alpha emitter Beta emitter New Isotope Thanks to D. T. Joss

Many nuclei at or beyond proton dripline are unstable against proton emission. Initially, parent nucleus is in a quasi-stationary state, and proton decay may be considered as a process where the proton tunnels through a potential barrier. Large Coulomb potential and centrifugal barrier mean this can often extend out to almost 100 fm. Consequently, measurement of decay half-lives (ranging from microseconds to seconds) provides reliable spectroscopic information. In principle, proton decay should be easy to model (since no preformation factors like alpha particles). Reviews: Experimental: Woods and Davids, Ann. Rev. Nucl. Part. Sci. 47 (1997) 541 Theoretical: Delion, Liotta and Wyss, Phys. Rep. 424 (2006) 113.

Spherical Nuclei Proton decay involves tunnelling through the potential barrier Total potential consists of nuclear + coulomb + centrifugal parts. The nuclear part is typically a mean-field potential and one has many choices of potential to take

WKB WKB is a semi-classical approximation. Inside nucleus, particle moves in classical-like orbit. Each time the barrier is hit, there is a probability that penetration will occur. The width and half life are given by where f is knocking frequency (with which the proton hits against the potential wall). The potential V(r) is felt by the proton and calculated by various means – e.g. Hartree Fock potential. It can also be used to estimate f. In the limit of constant potential inside the nucleus, the knocking frequency is based on a classical proton velocity and the nuclear radius: Or: Z.A. Dupre and T.J. Burvenich, Nucl Phys A 767 (2006)

Quasistationary picture Nuclear decays are time-dependent processes. However, typical decay lifetimes v. long on nuclear timescale => stationary state problem (Gamow 1928). Usually treated as scattering problem (poles in S-matrix or resonances in scattering amplitude). This is the time reverse of decay, that is wave comes in from infinity and becomes trapped by potential. However, quasistationary states of interest here might be closer to bound states (despite having continuous rather than discrete spectrum). Can use perturbative method reliably by starting from bound state problem.

Two-Potential approach Alternative method is known as the Two Potential approach (TPA). This is a fully quantum method, using perturbation theory developed by Shmuel Gurvitz. S.A. Gurvitz and G Kalbermann, Phys. Rev. Lett. 59 (1987) 262 S. A. Gurvitz, Phys. Rev. A 38 (1987) 1747 S. Åberg, P. Semmes and W. Nazarewicz, Phys. Rev. C 56 (1997) 1762 S. A. Gurwitz, P.B. Semmes, W. Nazarewicz and T.Vertse, Phys. Rev. A 69 (2004) 042705

 TPa: Outline V(r) = U(r) + W(r) ~ U(r) V(r) R r1 r2 R r W(r) W(r) R Quantum Method - using perturbation theory. V0  R r R r -V0

TPA: Theory Consider the unperturbed bound state in the potential U(r) with eigenvalue E0 : The perturbation, W (r) transforms it to a quasistationary state. When the potential is switch on at , the state becomes the wavepacket and we can derive a simple expression for the decay width Scattering wfn due to potential W(r) Radial bound state wfn in potential U(r) ~

TPA: Theory Since R is deep inside barrier, both bound and scattering states are simple exponentials in this region: R

TPA: Theory This allows the integral to be solved exactly: And a final simplification can be made to the scattering wave function outside the influence of the nuclear potential: Since the phase shift is so small inside the barrier, the second term above is negligible and to a good approximation Thus, S. Åberg, P. Semmes and W. Nazarewicz, Phys. Rev. C 56 (1997) 1762

Results Proton half-lives for various proton emitters calculated within the WKB and TPA models using a Hartree-Fock potential based on the SkP Skyrme force and compared with the measured values.

Summary for Spherical Emitters Proton emission using spherical potentials with WKB or TPA give reasonable results and in close agreement In principle, HF mean field potential provides proton energy too. In practice, the potential has to be scaled slightly to give correct proton energy. Underlying mean field cannot predict single particle energies sufficiently well.

Deformed proton emitters Currently several models on market to calculate partial decay widths for deformed nuclei: Gamow states method in adiabatic limit (complex energies) E. Maglione, L.S. Ferreira & R. J. Liotta, Phys Rev Lett 81 (1998) 538 Coupled Channels method (real energies) H. Esbensen & C. N. Davids, Phys Rev C 63 (2000) 014315 Both start from scattering state picture. e.g. first method: Partial decay width to proton channel is given by radial probability flux through a sphere of radius R outside the nuclear potential Proton single particle wave function in deformed potential Coulomb functions

TPa for deformed potentials As an alternative approach, can develop TPA in 3-D: For a deformed potential, barrier width now has angular dependence S1 and S2 denote equipotential lines for a proton with energy E0 Instead of a cut-off radius we now Have a separation surface, Σ, dividing the potential into inner and outer regions as before: S1 Σ S2 Shaded area is classically forbidden region

TPA for deformed potentials We then proceed as in 1-D case. [This has been developed by Gurvitz in Multiple Facets of Quantization and Supersymmetry: Michael Marinov Memorial Volume, Ed. by M Olshanetsky, A. Vainshtein] We obtain then a proton partial decay width where we have used the divergence theorem to give a surface integral. This needs to be solved with correct angular momentum projection onto decay channel.

Summary and Acknowledgements It is hoped that the 3-D TPA model of Gurvitz can be applied to study the single proton emission from deformed nuclei and compared with existing scattering state methods. This study formed part of a project with Paul Stevenson at Surrey, Robert Page and Dave Joss at Liverpool and John Simpson at Daresbury.